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SUMMARY:The Dark Matter distribution of the Milky Way (its astrophysical u
 ncertainties and effects on determination of physics beyond the standard m
 odel)
DTSTART;VALUE=DATE-TIME:20191112T050000Z
DTEND;VALUE=DATE-TIME:20191112T053000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182616Z
UID:indico-contribution-431-46@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Iocco\, Fabio (Imperial College / Università di Nap
 oli)\nThe distribution of Dark Matter in galaxies is one remarkable output
  of structure formation in a cosmological context\, and an important input
  for the searches of the nature of Dark Matter. In this talk I will presen
 t the results of recent\, fully data-driven analysis of the determination 
 of the Dark Matter content and distribution in the Milky Way. \nI will als
 o highlight the current uncertainties of empirical (and astrophysical) nat
 ure\, and how they affect the interpretation of direct and indirect search
 es\, and eventually the searches for the very nature of the Dark Matter.\n
 \nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1525/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1525/
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SUMMARY:Varieties of DM density profile in Galactic dwarf spheroidal galax
 ies and the gamma-ray search of the annihilation signature
DTSTART;VALUE=DATE-TIME:20191112T053000Z
DTEND;VALUE=DATE-TIME:20191112T060000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182616Z
UID:indico-contribution-431-64@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Hiroshima\, Nagisa (Riken)\nDwarf spheroidal galaxie
 s (dSph) are good targets to search for dark matter annihilation signals t
 hrough gamma-ray observations. Currently\, the most strong constraints on 
 the cross-section at mDM\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/co
 ntributions/1538/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1538/
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BEGIN:VEVENT
SUMMARY:Paradigms and Scenarios for the Dark Matter
DTSTART;VALUE=DATE-TIME:20191112T043000Z
DTEND;VALUE=DATE-TIME:20191112T050000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182616Z
UID:indico-contribution-431-83@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Salucci\, Paolo (SISSA)\nThe deeper we go into the k
 nowledge of the dark component that embeds the stellar component of galaxi
 es\, the more we realize the profound interconnection which is  present be
 tween the two of them. The scaling laws among the structural properties of
  the dark and luminous matter in disc systems are too complex to be arisen
  by two inert components that just share the same  gravitational field. Th
 is brings us to critically focus on the 30 years old paradigm\, that\, res
 ting on a priori knowledge of the nature of dark matter (DM)\, has led us 
 to a restricted number of scenarios for dark matter. The galaxies's struct
 ural properties show strong indications that the dark and luminous compone
 nts have interacted in a direct way over the Hubble time. We propose to br
 eak the dark matter mystery by taking a step back and start following a ne
 w paradigm: the Nature of dark matter can be guessed/derived only from dee
 p analyzing the properties of the dark and luminous mass distribution at g
 alactic scales. As first result in Spirals\, the quantity $\\rho_{DM}(r\,L
 \,R_D) \\rho_\\star (r\,L\,R_D)$\, the (macroscopic) kernel of a dark-to-l
 uminous interaction\, shows specific properties that call for a collisiona
 l nature of the dark particle.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/
 259/contributions/1668/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1668/
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